Using Superfit (Howell et al. 2005, ApJ, 634, 1190) and SNID (Blondin & Tonry 2007, ApJ, 666, 1024), we find several good fits to normal SNe Ia approximately two weeks after max. The redshift range reported in the fits is consistent with the NED value of the redshift for the probable host (2MASS J15503740+2302488; z = 0.115759). Assuming this redshift and distance modulus, the peak g-band absolute magnitude in the ZTF lightcurve is approximately -19.3. The absolute magnitude and the epoch of the spectrum are consistent with a post-max SN Ia.

The blue continuum with the possible HeII 4686 and NIV 4537 flash features suggests a very young Type II. The redshift measured from the narrow host Hα and [OIII] emission lines in the 2D spectrum agrees with the host redshift on NED (0.018150; 2006AJ….132..231P).